The galaxy presents a generally smooth, elliptical morphology. It exhibits a concentrated central bulge that gradually fades outwards. The galaxy's color profile appears relatively uniform, suggesting an older stellar population dominated by evolved stars. There is no readily apparent disk structure or spiral arm features. The overall shape tends towards a slightly flattened spheroid, falling between a perfectly round form and a more elongated shape. There are no obvious signs of tidal disturbances, major mergers, or significant ongoing star formation activity from visual inspection alone. Any faint disturbances or structures cannot be distinguished from the image resolution. The galaxy's relatively redder color indicates a quiescent state and a higher mass.
