The galaxy presents as a concentrated, centrally-bright object with an overall smooth appearance. It exhibits a nearly circular morphology, showing minimal elongation. A slight color gradient is visible, trending towards redder hues in the central region, indicative of an older stellar population and dust obscuration, and bluer hues on the outskirts, hinting at more recent star formation. There is a lack of prominent spiral arm structure or other distinct features within the galaxy's disk. A subtle diffuse halo may be present, but it is difficult to distinguish due to the image resolution. There is no obvious evidence of tidal disturbances, major mergers, or interacting companions in this image.
