This galaxy appears as a moderately bright, somewhat elliptical object. Its color profile suggests a relatively evolved stellar population, leaning towards redder hues, possibly indicating older stars. Although the galaxy appears relatively smooth in structure, there may be slight irregularities in its shape. Its moderate luminosity suggests it is a massive galaxy, and its star formation rate is likely to be higher than average. The galaxy appears relatively isolated and does not obviously seem to be in the process of merging.
