The galaxy presents as a relatively compact, elongated structure. The central region exhibits a bright, concentrated luminosity, suggestive of a prominent galactic nucleus and/or a significant bulge component. The overall color is primarily yellowish-red, hinting at a stellar population dominated by older, redder stars. There is a faint, extended disk component with some visible structure, although the resolution limits a detailed assessment of spiral arms or other features. A very subtle hint of bluer light can be observed in some regions, possibly indicating localized star formation, although this is not a dominant characteristic. The shape appears to be somewhere between elliptical and spiral, leaning more towards the elongated shape. Signs of recent major merger events are not evident in the images, but some disturbances could be suggested. 
