The galaxy presents as an apparent elliptical morphology. It exhibits a bright central bulge, which decreases in luminosity towards the outer regions. The central region displays a concentrated, bright core. The galaxy appears to be relatively smooth in texture. There is a slight hint of asymmetry or disturbance to the left, that looks like a "tail" with relatively less defined and slightly disrupted features, which could indicate possible tidal interactions or minor merger activity. Based on color gradients, the central bulge seems to be dominated by older stellar populations, based on its redder color, while the outer disk has a slightly bluer hue, potentially indicating areas of ongoing or recent star formation. Overall, the galaxy does not show strong evidence of spiral arms or a well-defined disk structure.
