The galaxy presents a largely smooth and elliptical morphology. The core region is dominated by a bright, relatively uniform yellowish glow, suggesting a population of older stars. There appears to be minimal evidence of spiral arm structure or prominent dust lanes. The galaxy appears roughly circular in shape, lacking any significant elongation or tidal distortions. The overall color profile indicates a lack of significant ongoing star formation. The light distribution is concentrated towards the center, with a gradual decrease in intensity outwards. Faint, diffuse extensions can be observed, though they do not appear to be associated with any major merger events.
