The galaxy appears as a centrally concentrated object with a generally smooth morphology. The light distribution suggests a moderate degree of central concentration, without evidence of distinct spiral arms or a prominent bar structure. The isophotes are mostly elliptical, with a slight deviation towards a more irregular shape. There is some faint structure suggestive of a disk, but the galaxy is generally featureless. The color profile indicates a relatively homogenous stellar population. The galaxy does not show any obvious signs of ongoing major merger activity, although subtle disturbances cannot be ruled out at this resolution.
