The galaxy in question presents a generally smooth and elongated morphology. It exhibits a reddish hue, suggesting an older stellar population and lower ongoing star formation rate. The galaxy appears to lack prominent spiral arm structures or a distinct central bulge. Its shape is more akin to a cigar or elliptical form, with the major axis significantly longer than the minor axis. There's no obvious evidence of a major merger event or significant tidal disturbances. The overall structure suggests a relatively evolved system dominated by older stars.
