The galaxy presents as a luminous, fairly symmetrical elliptical type. Its central region exhibits a high surface brightness, gradually diminishing towards the outer edges. The colour profile suggests a relatively uniform distribution of older stellar populations across the galaxy, with a hint of redder hues. There is little to no evidence of active star formation regions or prominent spiral arms. The overall smoothness and lack of significant morphological disturbances indicate a dynamically relaxed system, and it shows no obvious signs of ongoing or recent mergers. The galaxy appears isolated, with no visually interacting companions nearby.
