This galaxy exhibits a generally smooth morphology with a discernible, elongated shape. The central bulge appears prominent and is characterized by a yellowish-gold hue, suggestive of an older stellar population. Extending outward from the core, a bluer component is observed, which is likely indicative of more recent star formation within a disk-like structure. The overall shape is cigar-like and moderately inclined with respect to our line of sight. There is no obvious presence of spiral arms, a bar structure, or any signs of major disturbances related to on-going or recent galaxy mergers. Faint extensions or tidal features are not readily apparent, suggesting relative gravitational isolation and an undisturbed evolutionary history.
