The galaxy appears as a moderately luminous, elongated structure. The central bulge exhibits a concentrated, smooth, yellowish-orange hue, suggesting an older stellar population. Fainter, bluer light extends from the central region towards the outer edges, possibly indicative of ongoing star formation within a disk component. The galaxy's shape is cigar-like, implying it may be an elliptical galaxy or a spiral galaxy viewed edge-on. There are some minor disturbances to the structure, likely due to a potential interaction with another galaxy, but it does not appear to be a major disturbance or merger.
