The galaxy appears to be an elliptical or lenticular galaxy, exhibiting a smooth, largely featureless morphology. The light distribution is concentrated towards the center, with a radial falloff in intensity. There is little evidence of spiral arms or dust lanes. The galaxy presents a generally rounded appearance, with a slight elongation. The color gradient suggests a population of older stars, with a reddish-yellow hue dominating the central regions. There is no clear indication of ongoing major merging events or significant disturbances in its structure, although there may be a very faint and subtle asymmetry present in the outer regions. Overall, the galaxy gives the impression of a relatively relaxed and evolved system.
