The galaxy appears to be a relatively compact and luminous system. It exhibits a smooth, elliptical morphology, with a centrally concentrated bulge that shows some signs of active star formation. The overall color profile suggests a population of intermediate-aged stars, along with traces of younger, hotter stars contributing to the blueish halo. There appears to be a lack of significant dust lanes or tidal features, indicating that it has likely experienced no recent major merger events. The galaxy exhibits an overall smooth structure, with no obvious indications of a disk or spiral arms. The galaxy's roundness suggests that it is viewed close to face-on.
