The galaxy presents a largely smooth morphology, with little evidence of significant spiral structure or distinct features. The overall shape appears somewhat elliptical, though it tends towards roundness rather than a highly elongated form. There are no visible signs of a major ongoing merger or significant tidal disruption. Subtle irregularities in the outer regions may indicate minor gravitational disturbances or interactions, though these are not overtly prominent. Color gradients suggest a relatively older stellar population, with a central region appearing more yellow or reddish. The central region appears to be relatively concentrated, and the galaxy displays no prominent dust lanes or knots of star formation. The galaxy displays a moderately bright core that dominates the overall luminosity profile.
