The galaxy presents as a relatively faint, compact object. Its morphology appears largely spheroidal, exhibiting a smooth, diffuse light distribution without prominent spiral arms or a distinct disk structure. There is a slight color gradient, trending towards bluer hues in the central region, implying the presence of younger stellar populations compared to the outer regions. However, overall color is intermediate between red and blue suggesting the presence of both old and younger stars. There is no indication of active galactic nuclei activity. There is no evidence of tidal tails, or other signs of mergers. Based on its appearance, the galaxy is likely a low-mass system. The galaxy exhibits a minimal level of internal structure.
