The galaxy presents as an elliptical or lenticular system, exhibiting a smooth, diffuse light distribution with a noticeable central bulge. The overall shape is elongated, implying a non-spherical structure. There is a slight color gradient visible, with a yellow-orange hue concentrated in the central region, suggesting an older stellar population. Fainter blue hues are observed in the outer regions which may indicate younger stars or star forming regions. There is little to no evidence of distinct spiral arms or prominent dust lanes. Faint light disturbances possibly indicate tidal interactions or minor mergers.
