The galaxy presents as a dominant elliptical form, exhibiting a smooth, centrally concentrated luminosity profile. The primary body of the galaxy appears slightly elongated, but not markedly cigar-shaped. There is an apparent absence of spiral arm structures or prominent dust lanes. The color gradient shifts from a yellow-white core to a reddish-orange outer halo. This is suggestive of an older stellar population dominating the overall light output, with possible recent star formation, though at a low rate. The outer regions exhibit signs of minor disturbances or potential interactions, with a faint asymmetric glow in the upper regions. It seems unlikely to be undergoing a major merger event, however, it cannot be ruled out completely. A smaller, distinct object of relatively similar color and brightness is observed at a short angular distance from the main galaxy. This nearby object can potentially be a satellite galaxy of the main object. Overall the system seems to have high mass.
