The galaxy presents as an elliptical or lenticular type, displaying a generally smooth and concentrated light profile. There is little evidence of spiral arms or significant dust lanes. The central bulge is prominent and appears spheroidal in shape. The color gradient suggests an older stellar population, with a yellowish-red hue dominating the galaxy's overall appearance, particularly towards the core. There is some bluer light in the surrounding area. The galaxy's apparent ellipticity is moderate. The galaxy appears relatively isolated, showing no signs of major tidal disturbances or ongoing mergers, although a slight asymmetry in the outer regions may indicate a past minor interaction or accretion event. Overall, the galaxy appears to be a relatively quiescent system, possibly nearing the red sequence.
