The galaxy presents as a single, relatively smooth object with a predominantly elliptical morphology. Its color profile is dominated by warmer tones, with a concentrated yellowish-orange hue suggesting an older stellar population. Faint greenish-blue tinges are visible on the periphery, indicative of possible regions of ongoing or recent star formation, though these are not prominent. The object is largely symmetrical with no clear evidence of spiral arms, bars, or significant tidal disturbances. The light distribution appears centrally concentrated, and the galaxy exhibits a high degree of roundness, with a lack of elongation. The absence of morphological peculiarities suggests that the galaxy is not currently undergoing a major merging event, and is likely in a relatively quiescent phase of its evolution.
