The galaxy presents an elliptical morphology, exhibiting a smooth, largely featureless structure. The light distribution suggests a spheroidal shape, with the luminosity concentrated toward the center, resulting in a bright, diffuse core. A gradual decrease in surface brightness is observed moving outward from the core. There is evidence of possible disturbance, with an irregularity that may be a tidal feature resulting from gravitational interaction, or an overlapping galaxy in the line of sight. The galaxy displays a color gradient, shifting from a bluer central region to redder outskirts. This could be indicative of older stellar populations dominating the outer regions, or dust obscuration within the central area. Star formation appears to be low, with no prominent HII regions or strong indicators of ongoing star birth. 
