The galaxy presents as a relatively smooth, elliptical structure with a notable lack of distinct features. The light distribution appears concentrated towards the center, indicating a prominent bulge. The overall shape is elongated, leaning toward an elliptical morphology rather than a perfectly circular one. Color gradients are subtle, with a yellowish hue dominating the central region, potentially indicative of an older stellar population. Fainter bluish or greenish tints are observed in the outer regions. There appears to be no clear evidence of spiral arms or dust lanes. The galaxy shows no obvious signs of ongoing merging activity or major disturbances.
