The galaxy presents as a somewhat smooth, disk-like structure. It appears elongated, exhibiting a moderate cigar shape. There is little evidence of major merging activity or strong tidal disturbances. A subtle asymmetry can be observed, possibly indicative of a minor interaction or internal dynamic process. The galaxy appears to be largely smooth with a faint, yet noticeable bluish tinge in the center, suggesting at least some level of recent or ongoing star formation. Overall, the galaxy seems to be a relatively undisturbed system, potentially in an intermediate stage of morphological evolution.
