The galaxy presents a predominantly smooth and rounded morphology, with a minimal presence of distinct features such as spiral arms or bars. The overall light distribution appears centrally concentrated with a gradual fall-off towards the edges. The galaxy exhibits an orange-yellow hue towards the center, potentially indicating an older stellar population and/or the presence of dust. There is a slight hint of bluish light toward one edge, hinting at ongoing or recent star formation in that region. Overall, the galaxy appears isolated, without any clear signs of ongoing major mergers or tidal disturbances, although minor interactions cannot be ruled out based on this single image. The galaxy has an estimated physical size of approximately 5 kpc in radius.
