The galaxy presents as a generally smooth object, with a centrally concentrated bulge. The light distribution appears to be moderately elliptical in shape, but trending towards a more round appearance. There is little evidence of distinct spiral arm structure or a well-defined disk. The core of the galaxy appears yellow, transitioning to a bluish hue in the outer regions. This color gradient could indicate ongoing star formation in the outer areas. No obvious signs of a major merger or significant tidal disturbances are visible; however, it is possible there is some minor interaction occurring. The galaxy is relatively compact.
