The galaxy appears as a centrally concentrated object with a somewhat elongated morphology. It exhibits a relatively smooth light distribution, with the majority of its luminosity concentrated in the core region. The color profile suggests a redder population of stars dominating the central region, gradually transitioning to slightly bluer hues towards the outer regions. There are faint signs of possible disturbance in its outer shape or faint tidal features, possibly indicating past interactions. However, based on the data, we are more likely to consider the galaxy undisturbed. The galaxy appears to be a relatively massive and mature galaxy, with signs of ongoing though not vigorous star formation.
