The galaxy appears to be a somewhat elongated, disk-shaped system, oriented at an angle relative to our line of sight. The central bulge is pronounced and exhibits a bright, yellowish-white color, suggesting an older stellar population. The disk component is less clearly defined but shows a bluer hue in comparison to the central region, which indicates the presence of some younger stars and ongoing star formation, albeit at a relatively low rate. The galaxy has a fairly smooth overall appearance with no clear sign of spiral arms or bar structure, and no major disturbances.
