The galaxy presents as a generally smooth, centrally concentrated object. The core region exhibits a brighter, more yellowish hue, suggestive of an older stellar population. The light distribution decreases steadily from the center outwards, with no distinct spiral arm structures or prominent dust lanes visible. There is a faint, extended halo or envelope surrounding the core. The overall shape appears elliptical. It is not perfectly round but more closely so than cigar-shaped. No strong signs of tidal disturbances or major mergers are apparent, though subtle features might be present.
