The galaxy presents as an elongated, disk-shaped structure with a noticeable central bulge. The bulge exhibits a yellowish hue, suggesting an older stellar population. The disk appears to be inclined relative to our line of sight, contributing to its observed elliptical shape. The outer regions of the disk show a bluer tint, possibly indicating the presence of younger, hotter stars and ongoing star formation. There is little to no apparent spiral arm structure visible in the image. The galaxy appears relatively smooth in texture, with no obvious signs of major disturbances or interactions. The light distribution is concentrated towards the center, gradually diminishing towards the edges.
