The galaxy presents as a relatively compact object with a smooth, centrally concentrated light distribution. Its shape appears to be somewhere between round and elliptical, with a hint of elongation but no obvious disk structure. The color profile suggests a population dominated by older stars, exhibiting a redder hue. The galaxy does not show any signs of significant ongoing star formation or recent merger activity, instead presenting a fairly quiescent morphology. No distinct spiral arms, bars, or other prominent features are apparent, which reinforces the conclusion that this is an older system.
