This galaxy presents as a relatively smooth, elliptical structure. The light distribution is centrally concentrated, displaying a smooth gradient outwards from a brighter, somewhat diffuse core. The shape is elongated, exhibiting a cigar-like form rather than a perfectly circular appearance. There is a subtle color gradient; the central region appears slightly more yellow-green, potentially indicating a population of older stars, while the outer regions show hints of redder hues. No distinct spiral arm structures or significant dust lanes are discernible. There may be some indication of minor disturbances in the galaxy, though overall, it is likely an older galaxy with reduced star formation.
