The galaxy presents a relatively smooth and rounded morphology. There is no distinct spiral arm structure or bar visible in the image. The light distribution appears centrally concentrated, indicative of a substantial bulge component. The color profile suggests a dominant population of older stars, as evidenced by the redder hues. However, the presence of some bluer regions indicates ongoing, albeit modest, star formation activity. There are no obvious signs of major merger events or significant tidal disturbances in its immediate vicinity, although there may be a minor disturbance. Overall, the galaxy appears to be an evolved system transitioning towards a passive state. The estimated physical size of the galaxy appears to be large relative to the objects around it, but not overly large.
