The galaxy appears as a centrally concentrated object with a somewhat elongated morphology. It presents a relatively smooth appearance, suggesting a lack of prominent spiral arm structures. There is faint evidence of a disk-like structure with only subtle features. The color profile indicates a moderately evolved stellar population, with more light emitted at the redder end of the spectrum. A slight asymmetry may suggest minor tidal interactions. Overall, the galaxy appears to be an intermediate mass system at a considerable distance.
