This galaxy presents as a relatively smooth, elongated structure. Its color profile suggests a dominant population of older stars, indicated by the reddish-orange hue, though some blue light is present. There is little to no indication of spiral arm structures or active star formation regions from the imaging. The galaxy appears to be a near edge-on disk with an apparent cigar-shaped morphology. No major merger events or significant tidal disturbances are evident. A slight central bulge is noticeable, but it does not dominate the overall morphology. There is no prominent dust lane visible. Overall, the galaxy likely represents a fairly massive, evolved system with a relatively low specific star formation rate.
