The galaxy presents a morphology consistent with an elliptical type, exhibiting a generally smooth and concentrated light distribution. There is a notable absence of distinct spiral arm structures or prominent dust lanes. The galaxy's overall shape appears to be moderately elongated rather than perfectly spherical, with a suggestion of being in between round and cigar shaped. The central region is the brightest, indicating a concentration of stars toward the core. There is no readily apparent evidence of major mergers or significant tidal disturbances affecting the system. The color profile suggests a population of older stars, as indicated by the apparent yellowish-red hue and the absence of bright blue regions associated with active star formation. There may be a very slight indication of a minor disturbance that is causing a bit of asymmetry in the outer halo of stars.