The galaxy presents a primarily smooth morphology, suggesting a dominant spheroid component. Its overall shape is elliptical, appearing somewhat elongated with a cigar-like profile. A bright, concentrated central bulge exhibits a yellowish-white hue, indicative of an older stellar population. Fainter, reddish-orange light extends outward from the core, potentially tracing evolved stars within the galaxy's halo or disk. There is little evidence of prominent spiral arm structures or significant dust lanes. Based on its apparent color and form, the galaxy likely has a low specific star formation rate. Any signs of tidal disturbances or ongoing mergers are subtle.
