The galaxy presents as an elongated, cigar-shaped structure. It displays a smooth, diffuse morphology with a central bulge that appears to be the most luminous region. A faint disk is suggested by the subtle flattening. The galaxy exhibits a color gradient, transitioning from a yellowish-orange core towards a bluish hue in its outer regions. There is no obvious presence of spiral arms, bars, or other distinct features within the disk. The smooth appearance indicates that the galaxy is likely a relatively quiescent system, possibly an early-type galaxy. Evidence of any major disturbances or ongoing merging events is not apparent. The colors suggest the presence of both older stellar populations in the core and younger, star-forming regions in the periphery.
