The galaxy presents as a relatively compact and luminous object. Its morphology is smooth, with no apparent spiral arms or bar structures discernible. The color profile indicates a likely evolved stellar population, with a yellow-orange hue suggesting a dominance of older, redder stars and lower levels of ongoing star formation. The light is centrally concentrated, and the shape appears mostly round. There are no signs of significant tidal disturbances or ongoing major mergers. The galaxy does not appear to be undergoing any active merging activity. The galaxy shows signs of minor disturbances. Overall, this galaxy likely represents a massive, quiescent system that has largely exhausted its gas reservoir for star formation.
