The galaxy presents as a somewhat smooth, centrally concentrated object. It exhibits a general elliptical morphology with a diffuse halo or extended envelope. The core region appears brighter and more uniform in color, suggesting an older stellar population, while the outer regions show hints of less structured light, possibly indicating more recent or ongoing minor disturbances. The galaxy displays a yellow to orange hue in its central region, indicative of a population of older, redder stars and little active star formation. There are faint, possibly merging, arms or plumes on the edges of the galaxy, these features would be indicative of minor tidal interactions. Overall, the galaxy appears to be in a relatively quiescent state, with little evidence of active star formation or major disturbances.
