The galaxy presents as a moderately bright, elongated system. The light is dominated by a smooth central bulge, exhibiting a yellowish-white hue, which suggests an older stellar population. Extending outwards from the bulge is a fainter disk component, slightly bluer in color. The overall shape appears somewhat irregular, with a cigar-like elongation rather than a perfectly rounded structure. There is no evidence of strong spiral arm structure or significant dust lanes visible in this image. The galaxy does not display any obvious signs of ongoing mergers or major tidal disturbances, though a slight asymmetry could indicate a minor interaction in the past.
