The galaxy presents a predominantly smooth, elliptical morphology. It exhibits a concentrated central bulge that transitions into a more diffuse outer halo. There is no apparent disk structure or spiral arm features visible in this image. The color profile suggests an older stellar population, with a yellowish-red hue indicative of evolved stars. There is no significant evidence of ongoing star formation regions or dust lanes. Overall the galaxy appears to be a relatively undisturbed system, exhibiting no signs of major merging or tidal interactions. The shape appears to be largely round. There is a possible minor asymmetry in the outer halo, but it is difficult to determine the nature of the cause of this asymmetry from this single image.
