The galaxy presents as a generally smooth, elliptical-like morphology. It exhibits a dominant central bulge region, with the light intensity gradually decreasing towards the outer edges. The color profile is primarily yellowish-orange, suggesting a population of older stars. There is little evidence of spiral arm structure or significant dust lanes. The galaxy does not appear to be undergoing any major merging events, and shows only minor disturbances, if any. It is a moderately large galaxy. Overall, the galaxy appears to be a relatively passive system.
