The galaxy presents as a centrally concentrated object with an overall elliptical morphology, though exhibiting a subtle degree of asymmetry. The color distribution suggests a dominant population of older stars, particularly within the central bulge, indicated by the reddish hue. Fainter, bluer regions are visible in the disk, potentially signifying areas of ongoing or recent star formation. The galaxy has an estimated size of roughly 16 kpc, corresponding to a moderately sized galaxy. There appear to be signs of some kind of interaction or recent merger in the form of disturbances in the central regions. The galaxy is likely a massive system with a relatively low star formation rate.
