The galaxy presents as an elliptical morphology. The light distribution appears smooth with no apparent spiral arm structure or prominent dust lanes. The radial surface brightness profile suggests a concentrated nucleus fading gradually outwards. The color appears yellowish-orange across the galaxy, suggestive of an older stellar population. There may be minor asymmetrical features hinting at a past merger event, but the overall structure is largely undisturbed. Given the color and morphology, this galaxy is likely experiencing relatively low star formation activity. The overall round appearance implies we are viewing it closer to face-on than edge-on.
