The galaxy presents as a fairly compact elliptical with a smooth light distribution and no visible spiral arm structure. It displays a relatively high central surface brightness that gradually fades outwards, appearing more concentrated near the core. The color profile indicates a redder hue, possibly suggesting an older stellar population and lower star formation rate. There is little evidence of dust lanes or patches. The galaxy appears slightly elongated. Overall, it exhibits a fairly regular morphology, showing no strong signs of tidal disturbance or recent merger activity.
