The galaxy presents as a luminous, elliptical-shaped structure with a smooth, largely featureless morphology. The central region exhibits a concentrated, bright core, suggesting a high density of stars. The galaxy's color profile appears to be dominated by yellowish-orange hues, indicative of an older stellar population. There is little to no evidence of significant spiral arm structures or prominent dust lanes. The overall smoothness and lack of distinct features indicate a relatively evolved system. There may be a faint extended halo or envelope surrounding the brighter central region, though the image resolution limits detailed analysis of its extent and properties. The galaxy appears relatively isolated, showing no obvious signs of ongoing major mergers or significant tidal interactions with nearby galaxies.
