The galaxy presents as a relatively smooth, centrally concentrated object. Its morphology appears elliptical, lacking prominent spiral arms or a well-defined disk structure. The light profile suggests a smooth transition from a bright core outward. The color appears to be generally red/yellow tinged, with the central region exhibiting a more intense yellow hue which indicates an older stellar population. There is no obvious evidence of ongoing major merging activity or tidal disturbances, although there may be very faint substructure in the outer regions.
