The galaxy appears to be a relatively smooth, elliptical-type galaxy. It exhibits a bright, concentrated central bulge, surrounded by a more diffuse halo. There is little evidence of spiral arm structure or significant dust lanes. The overall shape is quite round, displaying a smooth, featureless appearance. There may be some slight asymmetry or minor disturbance in the outer regions of the halo, potentially indicating a past or ongoing interaction, but the galaxy does not seem to be undergoing any major merging activity. Colors suggest it consists of an older stellar population, as indicated by its yellow hue. The galaxy's estimated size, suggests it is a moderately sized galaxy. Despite its smooth appearance, a subtle underlying structure or faint, unresolved features may be present, requiring higher-resolution imaging for further analysis.
