The galaxy presents as a relatively smooth, elliptical form. There is little discernible disk structure, and no prominent spiral arms are visible. The galaxy exhibits a centrally concentrated brightness profile, with the luminosity decreasing gradually towards the outer regions. Its overall shape is largely round. No major disturbances or signs of ongoing mergers are immediately apparent in its structure. The color appears to be intermediate, showing the presence of both older stellar populations and some younger, bluer stars. Given the apparent size, this galaxy is likely a moderate-sized object. The faintness suggests it is reasonably far away. The star formation activity is low, which contributes to the redder color.
