The galaxy presents as a relatively smooth, elliptical morphology. There is a high degree of central concentration of light, with a gradual decline in surface brightness moving outward from the core. No obvious spiral arm structure or prominent dust lanes are discernible. The overall shape is neither perfectly spherical nor highly elongated, tending toward a more intermediate elliptical form. There is a slight suggestion of minor asymmetry or a subtle tidal feature, but no clear evidence of a recent major merger or strong gravitational interaction. The galaxy's color appears generally redder than many spiral galaxies, indicative of an older stellar population and potentially lower ongoing star formation. Overall, the galaxy appears as a moderately massive, relatively evolved system.
