The galaxy presents as a singular, largely homogenous object. Its overall morphology appears to be elliptical, with a slight deviation from perfect circularity towards a more oblate shape. The light distribution is generally smooth and concentrated towards the center, suggesting an older stellar population. There is a subtle color gradient, shifting slightly redder towards the central region, potentially indicating a higher concentration of older, redder stars in the core. There is a lack of distinct spiral arms or prominent dust lanes visible. No strong tidal features or signs of recent merger activity are apparent, although there may be a slight asymmetry in the outer regions, possibly suggesting a past minor interaction. The object appears relatively undisturbed, with no clear evidence of a recent major merger event.
