The galaxy presents as a relatively smooth, elliptical-like object with a noticeable central bulge that appears slightly more luminous than its surrounding structure. The overall morphology leans towards an elongated, cigar-shaped form rather than a perfectly circular or disk-like structure. There appears to be a gradual decrease in luminosity from the core outwards, with no distinct spiral arms or prominent features typically associated with active star formation visible in this image. The galaxy's color profile suggests a population of older stars, with a tendency towards reddish hues throughout. There is no readily discernible evidence of significant tidal disturbances or ongoing merger activity in this view.
