The galaxy presents as a moderately bright, relatively compact object. It appears largely smooth in texture, with a predominantly elliptical morphology. The galaxy exhibits a generally round shape, with only minimal deviation towards an elongated or cigar-like form. There are no prominent features suggestive of a strong disk component.

A hint of internal structure is visible; subtle variations in luminosity across the galaxy's surface imply some level of inhomogeneity in its stellar population or dust distribution. The central region seems slightly brighter and more compact than the outer regions.

The overall color profile is consistent with an evolved stellar population. There is an absence of bright blue regions, suggesting a low rate of on-going star formation.

The majority of the galaxy appears undisturbed, with no clear signs of recent major mergers or significant tidal interactions. Some minor asymmetry, or faint extensions, might be present at the limits of detection. More data is needed to accurately establish the extent and features of this distant galaxy.
