The galaxy appears to be a relatively compact object, exhibiting a somewhat smooth, elliptical morphology. The color profile indicates a dominant population of older stars, with a reddish-orange hue. There is minimal evidence of spiral arm structure or significant dust lanes. A small, faint blue region is slightly offset from the galaxy's center, potentially indicating a small region of star formation. However, the overall star formation rate is relatively low. The galaxy shows no strong indications of a major merger event, although there is some potential for minor tidal disturbances. Its shape is mostly round with some cigar shaped features.
