The galaxy appears to be a lenticular or early-type spiral galaxy, displaying a prominent bulge and a relatively faint, elongated disk. The bulge exhibits a smooth, yellowish hue indicative of an older stellar population with minimal ongoing star formation. The disk component shows hints of bluer colors, possibly indicating some younger stars or regions of modest star formation, although these features are not very pronounced. The overall morphology is elongated and cigar-shaped, lacking distinct spiral arms or prominent dust lanes. There is no obvious evidence of recent major mergers or strong tidal interactions, with only a slight asymmetry suggesting possible past minor disturbances. The light distribution is relatively smooth across the galaxy, consistent with a system dominated by older stars.
