The galaxy appears as a centrally concentrated, elliptical-like object with a smooth, featureless morphology. The light distribution is brightest towards the core, gradually diminishing outwards, lacking any spiral arm structures or prominent dust lanes. The color profile indicates a redder hue, potentially suggestive of an older stellar population dominating its composition. There are no apparent tidal features or signs of recent merger activity observable at this resolution. The galaxy presents as relatively round in shape.
