The galaxy presents an elongated, cigar-shaped morphology. It exhibits a smooth, concentrated central bulge that dominates its overall structure. The color profile suggests an older stellar population residing within the bulge, appearing yellowish-orange. A faint, bluer disk component surrounds the bulge, contributing to a lower overall smoothness. There is no significant presence of spiral arms or distinct morphological features indicative of recent major mergers or significant star formation activity. The galaxy appears relatively undisturbed, with no apparent tidal tails or distortions in its overall shape. The galaxy does not appear to be undergoing a major merging event, but may be experiencing a minor disturbance.
