The galaxy presents as an elliptical morphology, exhibiting a smooth, centrally concentrated light distribution. Its overall shape is elongated, deviating from a perfectly circular form, and appearing somewhat cigar shaped. The galaxy's color profile indicates a dominant population of older stars, as suggested by the redder hues, particularly concentrated towards the central bulge. There is a subtle color gradient, with the central regions appearing more yellow. The galaxy shows little evidence of spiral arm structures or active star formation regions. No signs of significant tidal disturbances or ongoing merger events are apparent.
