The galaxy presents a generally smooth, elliptical morphology. The light distribution suggests a centrally concentrated luminosity profile, indicative of an older stellar population. The color is predominantly yellowish-orange, consistent with evolved stars and a lack of significant ongoing star formation. There is a slight asymmetry in the outer regions of the galaxy; a subtle extension of the light profile may indicate minor tidal interactions or past mergers. No distinct spiral arms or prominent dust lanes are visible. Overall, the galaxy appears as a relatively undisturbed, quiescent system.
