The galaxy appears as an elongated, roughly cigar-shaped structure. The central region exhibits a concentrated, brighter luminosity with a yellowish hue, suggestive of an older stellar population. Progressing outward from the core, the luminosity decreases gradually. The extended region presents a bluer color, potentially indicative of ongoing star formation within the galaxy's disk. No prominent spiral arm structures are discernible. The galaxy does not present any major signs of a merger, but does appear to have some minor disturbances. The galaxy presents as disk dominated, but also seems relatively smooth, which is consistent with an aging galaxy with reduced star formation. Overall, this galaxy seems to be a disk galaxy, and the observations suggest it is in the process of winding down it's star formation.
