The galaxy presents a generally smooth morphology, suggestive of an elliptical or lenticular type. There is no readily discernible spiral arm structure. The light distribution appears centrally concentrated, exhibiting a bright, diffuse core that gradually fades towards the outer regions. The galaxy's overall shape is elongated, but not significantly cigar-shaped. There's a subtle hint of asymmetry or minor disturbance in the outer envelope, but no clear evidence of major merging or tidal interactions. The color gradient indicates a redder hue in the central bulge, potentially indicative of an older stellar population, transitioning to slightly bluer tones in the outer regions, possibly due to the presence of younger stars or ongoing, but subdued, star formation.
