The galaxy presents as a single, largely homogenous, and moderately concentrated light source. The morphology is generally smooth, lacking any easily discernible spiral arms or prominent features. The central region exhibits a brighter, more intense coloration trending towards yellow and orange hues, indicative of an older stellar population. There's a slight color gradient moving outwards from the center, with colors gradually becoming fainter. The galaxy appears somewhat circular, hinting at a possible elliptical or lenticular classification. There appears to be very little active star formation, consistent with its color profile and smooth texture. No obvious signs of mergers or tidal disturbances are observed.
