The galaxy presents as a relatively smooth, centrally concentrated object. Its overall shape appears approximately elliptical, tending toward round, with minimal discernable structure within the main body. A bright, yellowish core region is apparent, suggestive of an older stellar population. The outer regions of the galaxy are bluer in color, indicative of possible ongoing or recent star formation activity. There is no obvious spiral arm structure or bar feature. No signs of major mergers or tidal disturbances are readily apparent, although some minor asymmetry or a subtle irregularity in the outer envelope cannot be entirely ruled out. The galaxy shows an appreciable size, corresponding to an absolute magnitude indicating a significant luminosity. The moderate redshift implies a considerable distance, and a derived stellar mass suggests it is a massive galaxy. A low-to-moderate level of star formation is indicated by color and inferred star formation rate, classifying it as a galaxy on the red sequence.