The galaxy presents a smooth, elliptical morphology, exhibiting a centrally concentrated luminosity profile. The galaxy core appears bright, with a gradual decrease in luminosity towards the outer regions. There is no clear indication of spiral arm structure or a distinct disk component. The overall color appears to be redder, indicative of an older stellar population and potentially lower levels of on-going star formation. The isophotes exhibit a generally rounded shape, with no major signs of tidal disturbances or ongoing merger activity, though a slight asymmetry is visible. There may be a possible interaction with a second galaxy but more data is needed.
