The galaxy presents as a slightly elongated, disk-shaped system oriented at a high inclination relative to the observer's line of sight. The central bulge exhibits a bright, concentrated luminosity, appearing yellow to white in color, suggesting a population of older stars. Moving outwards from the center, the disk component displays a gradually decreasing luminosity. The outer regions of the disk show a subtle bluer tint, possibly indicating areas of ongoing star formation or a younger stellar population. The galaxy appears relatively undisturbed, showing no signs of major mergers or tidal interactions. It seems to be a relatively quiescent system with a moderate amount of star formation activity, primarily located within its disk.
