The galaxy presents an elongated, somewhat cigar-shaped morphology. A central bulge region exhibits a concentrated, yellowish hue indicative of an older stellar population. Surrounding the core, a fainter, bluish disk is discernible, with a smooth appearance. The disk’s color suggests the presence of ongoing star formation. No spiral arm structures or significant dust lanes are immediately apparent in this image. There is no readily visible evidence of tidal features or major disturbances indicative of recent mergers. However, given the relatively small scale of the image, minor interactions cannot be ruled out.