The galaxy presents an elongated, cigar-shaped morphology, suggestive of an elliptical galaxy viewed from a non-face-on angle. The light distribution appears smooth and centrally concentrated, exhibiting a gradual decrease in intensity from the core outwards. The central region of the galaxy is noticeably brighter and exhibits a yellowish hue, possibly indicative of an older stellar population. Fainter blue-ish tones are visible in the outer regions, which could possibly indicate the presence of younger stars or star forming regions. There appears to be no significant presence of spiral arms or dust lanes. The galaxy does not appear to be undergoing any major merging events or exhibiting any strong tidal disturbances.
