The galaxy presents as a centrally concentrated, likely elliptical or lenticular system. It exhibits a smooth, diffuse light profile with a prominent bulge region that dominates the galaxy's overall luminosity. The core of the galaxy shows a distinct yellowish hue, suggestive of an older stellar population with relatively low ongoing star formation. Moving outwards from the center, the galaxy fades gradually into the background, with hints of a more bluish or greenish tint in the outer regions which could indicate the presence of younger stars or faint spiral arm structures. The galaxy appears largely undisturbed, lacking any obvious signs of recent major merger events or tidal interactions with neighboring galaxies, although there is some slight asymmetry to the outer halo. The galaxy has a compact structure, as it appears relatively small in size.
