The galaxy presents as a centrally concentrated object with a generally smooth morphology. The light distribution is dominated by a bright, slightly elongated core, appearing nearly circular in projection. The central region exhibits a reddish-pink hue, possibly indicative of an older stellar population or dust obscuration. Surrounding the core is a more diffuse halo, transitioning into a bluish color. This suggests a presence of younger stars or ongoing star formation in the outer regions of the galaxy. There is a slight asymmetry or minor perturbation visible in the outer halo, hinting at a possible interaction or minor merger event in its past, although no significant tidal features are immediately apparent. Overall, the galaxy appears to be a relatively massive system with a moderate level of star formation activity.
