The galaxy presents as a moderately bright, elliptical structure. The central region exhibits a high surface brightness, appearing nearly uniform and featureless, suggesting a dense stellar population. Moving outwards from the core, a gradual decrease in surface brightness is observed. The galaxy's overall shape is elongated, exhibiting an axial ratio suggesting a classification between E4 and E6 on the Hubble sequence. Faint, diffuse extensions are visible along the major axis, hinting at tidal features or a larger, more diffuse halo. The color profile appears relatively uniform across the galaxy, with a slightly bluer hue in the outer regions compared to the core. This could indicate ongoing star formation, albeit at a low rate. There is no evidence of spiral arms or a prominent dust lane, lending further support to an elliptical classification. The smooth morphology and lack of significant disturbances suggest the galaxy has not undergone a major merger event recently.
