The galaxy appears to be an elongated, spindle-shaped system with a smooth, diffuse light distribution. The central region presents a noticeable concentration of luminosity, possibly indicating a bulge or a more densely populated core. The galaxy displays a relatively uniform color gradient across its structure, tending toward redder hues throughout its entirety. There's no apparent structure such as spiral arms or prominent dust lanes visible in this image. The overall morphology is suggestive of a later-type galaxy viewed edge-on, which is supported by the elongated, cigar-like shape. There is no visible evidence of any major tidal disruptions or ongoing mergers with other galaxies. It seems to be a relatively undisturbed, isolated system, though there may be evidence of slight disturbances.