The galaxy presents as a relatively smooth, disk-shaped object with an apparent oblate morphology. It exhibits a noticeable central bulge, characterized by a concentrated, bright luminosity indicating a higher density of stars. The disk component appears relatively thin, with a slight inclination to our line of sight allowing us to observe it from a shallow angle. There appears to be little to no presence of prominent spiral arms or distinct star-forming regions. The overall color profile suggests a stellar population dominated by older stars with a reddish hue, though a hint of blue near the edge of the galaxy disk may imply some recent star formation activity. The galaxy seems to be generally isolated, with no obvious signs of ongoing major mergers or significant tidal distortions.