The galaxy presents as a moderately bright, relatively compact object. Its overall morphology appears generally smooth, with a central concentration of light. There is a hint of a disk-like structure, but it is not strongly defined. The galaxy has a noticeable roundness to its shape, appearing neither particularly elongated nor perfectly spherical. There is no clear evidence of any ongoing major mergers or significant tidal disturbances affecting its overall form, but there may be some minor disturbances. Based on its color profile, which appears to be more prominent towards the redder end of the spectrum, the galaxy likely hosts a population of older stars, although there is also evidence of more recent star formation within the galaxy.
