The galaxy appears to be a relatively compact, elliptical system. Its light profile seems smooth and concentrated, with no obvious spiral arm structures or prominent dust lanes. The galaxy presents a nearly circular shape. The galaxy's color seems to be shifted towards redder wavelengths, suggesting a population of older stars and a relatively low rate of ongoing star formation. There might be a faint extended halo surrounding the main body of the galaxy, but this is difficult to discern with certainty. There's no immediately noticeable sign of any major ongoing merger events or strong tidal disturbances impacting the galaxy's morphology.
