The galaxy appears to be a relatively small, elliptical galaxy. It exhibits a smooth, featureless morphology with a concentrated central bulge. The light distribution is fairly even, with a gradual decline in intensity from the core outwards. The shape is generally round. No distinct spiral arms or bar structures are visible. The color index suggests a population of older stars, as the galaxy exhibits a yellowish hue. There is no prominent dust lane or sign of active star formation. There appears to be some minor disturbance visible in the light profile, potentially suggesting a gravitational interaction with a much smaller body. No signs of recent or ongoing major merger events are visible.
