The galaxy presents as a luminous, primarily smooth object with a slightly elongated morphology. Its core region exhibits a concentrated, bright emission. A subtle disk-like structure is potentially present, albeit not sharply defined. The color profile shows a redder central bulge that transitions into a bluer hue towards the outer edges. This color gradient suggests the presence of younger stellar populations in the galactic outskirts. There are some tidal disturbances with a possible merging event occurring as evidenced by the distorted morphology and the presence of nearby objects, with blue star forming regions visible.
