The galaxy presents as a largely featureless, elliptical morphology. Its core region exhibits a concentrated luminosity, with light intensity decreasing radially outwards. The galaxy appears nearly spherical, lacking a prominent disk structure or spiral arms. There is no obvious dust lane or significant evidence of active star formation regions, though some weak, diffuse features may be present upon closer examination. Color analysis suggests a predominantly older stellar population, exhibiting a redder hue overall. No significant signs of ongoing mergers or tidal disturbances are readily apparent in this image.
