The galaxy presents as a concentrated, elliptical-like structure with a bright central bulge that fades into an extended, less luminous halo. The color profile suggests an older stellar population, exhibiting a redder hue in the central regions, possibly indicative of a higher concentration of evolved stars. The overall form appears relatively smooth and undisturbed, without any obvious signs of spiral arms or significant tidal interactions. The galaxy is moderately elongated, displaying an axial ratio of approximately 0.66. There is no apparent disk structure, indicating that the galaxy is either viewed at a high inclination or, more likely, that it is a spheroidal galaxy.
