The galaxy presents as a relatively smooth, single structure with an elliptical appearance. A bright, concentrated central bulge is visible, surrounded by a more diffuse disk. The galaxy exhibits an overall yellow-white hue, suggesting an older stellar population. The disk appears somewhat flattened. There is no evidence of distinct spiral arms or significant dust lanes. The light distribution decreases gradually from the core to the outer regions, characteristic of a Sersic profile with a slightly higher central concentration. There is a slight asymmetry in the light distribution, but it does not indicate a major merger event.