The galaxy presents a generally smooth, elliptical morphology. There is a concentrated central bulge that appears yellowish, likely indicating an older stellar population. The surrounding halo is more diffuse and exhibits a slightly bluer color, suggesting the presence of some younger stars. The galaxy displays a lack of any spiral arm structure or significant dust lanes. There is little evidence of any major merger events or tidal disturbances impacting its shape or composition. Overall, this is likely a relatively massive and quiescent galaxy.
