The galaxy appears to be an elliptical galaxy, exhibiting a smooth, centrally concentrated luminosity profile. It has an overall yellowish hue, suggesting an older stellar population with relatively little ongoing star formation. The galaxy is moderately elongated, with a shape transitioning between round and cigar-shaped, presenting an intermediate ellipticity. No clear spiral arm structures or prominent dust lanes are visible. There may be some minor disturbances with a small chance of it being a merger, as the galaxy has no obvious major asymmetry or tidal features indicative of an ongoing or recent major merger event. Overall, the galaxy seems to be a relatively quiescent, early-type system.
