The galaxy presents as an elliptical morphology, elongated with an approximate axis ratio of 1:5, suggestive of an E5 classification. The central region exhibits a high surface brightness, indicating a dense concentration of stars, likely an older stellar population dominated by redder wavelengths. There is minimal evidence of spiral arm structure or dust lanes. The outer regions fade gradually, indicative of a smooth stellar halo. There is faint evidence of a diffuse disk component, possibly a faint disk with some irregularities on its furthest extent. There is little to no indication of ongoing star formation based on color, appearing mostly red and yellow. No signs of a major merger, but there is some asymmetry in the outskirts of the galaxy that suggests a possible tidal interaction or minor merger event in the past, more prominent on the rightmost edge.
