The galaxy appears to be a relatively smooth, elliptical system. It presents a centrally concentrated light profile, with a gradual decrease in surface brightness extending outwards. The galaxy's core exhibits a yellowish hue, possibly indicative of an older stellar population. Fainter, diffuse green extensions are observed surrounding the core and may indicate the presence of faint star forming regions. The overall morphology suggests a galaxy that is not currently undergoing any major merging events or significant tidal disturbances.
