The galaxy presents as a single, relatively smooth object. The light distribution suggests a spheroid-dominated morphology, with a high degree of central concentration. The galaxy is not perfectly circular, appearing slightly elongated. A central bulge appears to be the dominant feature, with a gradual decrease in luminosity moving outwards. The overall color appears to be on the redder side, suggesting an older stellar population and relatively low levels of ongoing star formation. There is no evidence of distinct spiral arms, bars, or significant dust lanes. No obvious tidal features or signs of interaction with other galaxies are apparent.
