The galaxy presents as a relatively smooth, elliptical or lenticular system. The central bulge is luminous and appears yellow-white, indicative of an older stellar population dominating this region. A disk component is discernible, though less prominent than the bulge; it is oriented at a slight angle to our line of sight. There's little to no evidence of spiral arm structure or significant dust lanes, suggesting a lack of ongoing, large-scale star formation. The outer regions of the galaxy fade gradually into the background, indicative of a large radius. No obvious tidal features or signs of recent merger activity are observed. It is moderately bright, suggesting proximity or a high intrinsic luminosity.
