This galaxy appears to be an elliptical galaxy, exhibiting a smooth, featureless morphology. It possesses a distinct elongated shape, indicating that it may be a type E4-E7 galaxy on the Hubble sequence. The central region exhibits a concentration of light, which fades gradually toward the outer edges. The galaxy has a yellowish-white hue, possibly indicative of an older stellar population that is dominated by redder stars and lacking in significant ongoing star formation. There is no visible evidence of spiral arms or a well-defined disk structure. There does not appear to be any evidence of tidal tails or other disturbances that would suggest a recent or ongoing merger event.
