The galaxy presents a generally smooth, elliptical morphology. It exhibits a concentrated central bulge, which appears to be a yellowish hue. The galaxy's overall shape is somewhat elongated, tending toward an "in between" roundedness. There is a notable lack of distinct spiral arm structure or prominent dust lanes. There is no strong evidence of significant merging activity, although it is possible that some minor disturbances are occurring. The galaxy displays a range of stellar populations. The bright central region suggests a significant population of older stars. It is a relatively massive galaxy. Overall, this galaxy appears to be a relatively evolved system, consistent with a relatively low star formation rate and a population dominated by older stars.
