The galaxy presents as a somewhat elongated, disk-shaped structure with a distinct central bulge. Its color is primarily a bluish-white hue, suggesting a significant population of relatively young, hot stars and ongoing star formation. The smooth texture of the galaxy with a lack of apparent spiral arm structure indicates that it's most likely a lenticular galaxy (S0) or a relatively featureless spiral galaxy undergoing a period of quiescence in star formation. A slight irregularity observed at one end of the galaxy hints at a possible minor interaction or disturbance. The galaxy exhibits a clearly defined central bulge, which appears brighter than the surrounding disk, indicating a relatively high density of stars in the nucleus. There is no visible dust lane, suggesting a relatively low dust content.
