The galaxy presents a somewhat elliptical morphology, appearing neither perfectly spherical nor highly flattened. A prominent central bulge region is visible, displaying a concentrated luminosity. The color profile suggests a relatively evolved stellar population, with a yellowish hue dominating the core, potentially indicating a prevalence of older, redder stars. Some bluer emission is also present, but it is much less pronounced and concentrated in a small area on one side of the galaxy.

There are subtle hints of possible disturbances or tidal features in the outer regions, but they are not distinct. The smoothness of the light distribution is relatively high, suggesting a lack of significant ongoing major mergers or intense star formation throughout the disk, although some degree of low-level star formation may be present in small portions of the galaxy. Overall, the galaxy appears to be in a relatively quiescent state.
