The galaxy presents as an elliptical morphology, exhibiting a smooth, centrally concentrated light distribution. The core is a bright, yellow hue, indicative of an older stellar population. The light gradually fades outwards towards the edges of the galaxy, displaying a faint, diffuse halo. There is no clear evidence of spiral arms or prominent dust lanes. There is little evidence of ongoing star formation. The galaxy appears relatively undisturbed, without major tidal features or signs of recent merger activity. Overall the galaxy has a fairly round shape, with no cigar shaped features. 
