The galaxy presents an overall elliptical morphology with a high degree of central concentration. The light distribution appears smooth, with no obvious spiral arm structure or prominent dust lanes visible in this image. The color profile suggests a population of older stars, trending towards a redder hue, but some bluer areas may be visible, indicating some ongoing, albeit minimal, star formation. It does not show any obvious signs of major tidal disturbance or ongoing mergers, though some slight asymmetry suggests the possibility of a minor interaction in its past. The galaxy appears relatively isolated, without any obvious companion galaxies in close proximity. The overall structure is compact, with a fairly well-defined edge, but it lacks a sharp, well-defined boundary and instead appears to fade gradually into the background.
