The galaxy presents as a roughly elliptical, smooth object with a concentrated central bulge. The light distribution appears centrally peaked, exhibiting a strong intensity gradient moving outward from the core. The galaxy exhibits a color gradient, with a yellowish core fading to a bluer hue further from the center, suggesting radial variations in stellar populations. The galaxy shape indicates it may be a spheroidal galaxy of significant mass. There is some asymmetry in the light distribution within the galaxy, which may indicate a past or ongoing interaction. There appears to be some evidence of tidal features, but these are subtle. Overall the galaxy appears fairly isolated, with no obvious companion galaxies nearby.
