The galaxy presents as a somewhat elliptical or disk-like structure, although its precise classification is partially obscured. The central region exhibits a brighter, yellowish hue, suggestive of an older stellar population. Surrounding this core, a more diffuse, greenish component is observed. This greenish tint may indicate regions of ongoing star formation or ionized gas. The galaxy appears relatively smooth overall, with no obvious signs of major disturbances, mergers, or strong tidal interactions. It is moderately inclined to our line of sight. The shape is somewhere in-between round and cigar shaped. 
