The galaxy presents as an elongated, cigar-shaped structure. It exhibits a smooth, largely featureless morphology. There appears to be a brighter, slightly more concentrated central region, suggesting a bulge. The galaxy's color is generally reddish-orange, potentially indicating an older stellar population and lower star formation rate. There is a subtle gradation in brightness from the central region outwards toward the edges. No spiral arms, dust lanes, or other distinct features are readily apparent. There is little to no evidence of recent or ongoing major merging activity. Minor distortions in the overall shape may suggest some interaction or minor disturbance.
