The galaxy appears to be a relatively smooth, centrally concentrated object. Its morphology suggests an elliptical galaxy, possibly of type E3 or E4 based on its observed ellipticity, which appears slightly elongated but not significantly so. The light distribution shows a gradual decline in intensity from the core outward. The core itself displays a yellowish-orange hue. The observed color suggests an older stellar population dominating the light output. The galaxy doesn't display any visible dust lanes, spiral arm structures, or other prominent features indicating active star formation. There may be evidence of faint tidal features, but not significant enough to say that it is currently merging.