The galaxy presents as a concentrated, largely featureless elliptical morphology. Its color profile suggests a dominant population of older stars, exhibiting a yellowish hue centrally, transitioning to slightly redder tones towards the outer regions. There is a high degree of smoothness in its overall structure, lacking any distinct spiral arm patterns or prominent dust lanes. The galaxy appears relatively isolated, without any obvious signs of recent or ongoing major mergers or tidal disturbances, although there may be minor asymmetry. Its elliptical shape appears nearly round, showing very little elongation.
