The galaxy appears to be a relatively smooth, lenticular or early-type spiral galaxy, seen at a moderate inclination. It exhibits a bright, concentrated central bulge, which appears yellowish-white, suggesting an older stellar population. The disk component is less prominent, with faint, diffuse blue-ish hues emanating from the outer regions, possibly indicating some ongoing star formation. The overall shape is elongated, more cigar shaped than circular, and there's no evidence of strong spiral arm structure, although there may be subtle signs of a weak disk. There is no obvious indication of any major ongoing merger event. Based on the apparent color and morphology, this galaxy is likely to have an intermediate stellar mass and relatively low star formation rate. There may be a slight asymmetry visible, possibly indicating a minor interaction.
