The galaxy presents as a centrally concentrated elliptical type. The core exhibits a bright, relatively uniform luminosity profile, indicating an older stellar population. Extending outwards, the galaxy gradually fades, with the isophotes appearing moderately elongated, suggesting a cigar-like shape. There are no obvious signs of spiral arm structures or prominent dust lanes. The galaxy appears relatively smooth and undisturbed, lacking any significant tidal features or signs of ongoing major mergers. The color profile suggests a redder hue, consistent with a population of older, cooler stars and limited current star formation. There might be some minor disturbances, however, it appears largely non-interacting.
