The galaxy presents as a centrally concentrated object with a somewhat elongated morphology. The core region exhibits a bright, diffuse glow, indicative of a high stellar density. There appears to be a transition in color from the central region outward, with the core displaying a slightly redder hue, possibly suggesting an older stellar population. Fainter, bluer components extend from the central region, forming a less-defined disk-like structure, hinting at possible ongoing star formation. There are no distinct spiral arms visible. The overall structure seems relatively smooth, though there are slight irregularities in the outer regions, possibly suggestive of minor interactions or internal disturbances. No significant merging activity is apparent, although a slight asymmetry could point towards past gravitational interactions. 
