This galaxy appears to be an elliptical type. It presents as having a smooth, largely featureless morphology with a centrally concentrated luminosity profile that diminishes outward. The core region is bright, with a yellowish-white hue, suggesting a high concentration of older stellar populations. Moving outwards from the core, a faint blueish tinge is observed, potentially indicative of a small population of younger, hotter stars, or perhaps weak ongoing star formation in the outer regions. There is no distinct disk or spiral arm structure visible. The galaxy appears relatively isolated, without obvious signs of major tidal disturbances or ongoing mergers, although subtle asymmetries or minor irregularities in the outer envelope cannot be entirely ruled out at this resolution. The galaxy has a moderately rounded appearance, somewhere between a perfect circle and an elongated cigar shape.
