The galaxy presents a generally smooth morphology, with a somewhat elongated, cigar-like shape. Its color profile appears reddish, indicating a stellar population that is likely older, with lower rates of ongoing star formation. There appears to be a primary central bulge that is significantly brighter and more concentrated than the more extended, fainter disk. No prominent spiral arm structure is discernible in this image; however, this is likely due to the image quality and/or the galaxy being an elliptical type. There appears to be no evidence of any major ongoing merger activity or substantial tidal disturbances. The galaxy is at an estimated distance indicated by its redshift. The inferred mass suggests that the galaxy is a typical galaxy. Overall, this galaxy appears to be a relatively quiescent, evolved galaxy.
