The galaxy presents as an elliptical or lenticular-type system, displaying a largely featureless morphology with a high degree of central concentration. The light profile appears smooth, exhibiting a gradual decline in intensity from the core outwards. Color gradients are subtle, with a yellowish-white hue dominating the central region, potentially indicating an older stellar population. There is a very slight elongation, more round than cigar shaped. The galaxy does not show any prominent spiral arm structures or dust lanes that are typically observed in spiral galaxies, nor does it appear to be undergoing a major merger. There are minor indications that it may be interacting or in the process of merging.
