The galaxy presents a largely smooth and featureless appearance, exhibiting a centrally concentrated luminosity profile that diminishes gradually outwards. Its shape is more akin to an elliptical or lenticular morphology rather than a spiral. A slight elongation is discernable, suggesting a deviation from perfect circularity, but the galaxy is generally rounded. No spiral arms, dust lanes, or other distinct features typically associated with actively star-forming galaxies are visible. The color appears relatively uniform across the galaxy's body, trending towards a yellowish-white, suggestive of an older stellar population with a low star formation rate. There is no evidence of any major mergers or significant tidal disturbances in its immediate vicinity. Minor disturbances cannot be excluded, though they are not clearly visible.
