The galaxy appears to be a relatively smooth, centrally concentrated elliptical galaxy, exhibiting a primarily spheroidal morphology. The light distribution is dominated by an elliptical bulge with a yellowish hue, indicating an older stellar population. There's no clear evidence of spiral arms or a prominent disk structure. The galaxy shows a high degree of central concentration, with the light intensity decreasing gradually from the core outwards. There is a slight elongation, but it generally appears fairly round. There are no significant signs of any major merging events or strong tidal disturbances, though there might be some minor asymmetry. There is no visible dust.
