The galaxy presents as a moderately elongated, cigar-shaped structure with a smooth overall appearance. The color profile is dominated by warmer hues, trending towards redder wavelengths. This suggests an older stellar population. There is no readily apparent dust lane or spiral structure. The object shows no signs of any major ongoing merger events, although the possibility of a past minor interaction cannot be ruled out based on the available imagery. The central region exhibits a slightly higher surface brightness than the outer regions, which fade gradually into the background sky. Overall, the galaxy appears to be an elliptical galaxy at a significant distance.
