The galaxy presents as an elongated, cigar-shaped structure. A prominent central bulge is visible, exhibiting a smooth and concentrated light distribution, suggesting an older stellar population. Fainter, somewhat diffuse extensions emanate from the central bulge, indicating a disk-like component. There appears to be little active star formation currently occurring within the visible regions of this galaxy. Indications are that this is not a merger event. The central bulge dominates the overall morphology, contributing to the galaxy's classification as likely to be a smooth feature.
