The galaxy presents an elongated, somewhat cigar-shaped morphology. Its light profile appears smooth, lacking any obvious spiral arm structures or prominent dust lanes. The central region exhibits a bright, concentrated core, suggesting a relatively high stellar density in the nuclear region. The galaxy's overall color is relatively uniform and indicative of an older stellar population, although the presence of some bluer regions might point to some ongoing, albeit low-level, star formation activity. No significant tidal features or signs of recent major mergers are readily apparent, suggesting it is a relatively isolated system that might be undergoing some minor disturbances.
