The galaxy presents a predominantly smooth, elliptical morphology. A concentrated bulge is apparent, exhibiting a yellowish hue, suggestive of an older stellar population. Fainter, bluer light extends outwards from the central bulge, possibly indicative of more recent, albeit subdued, star formation within the galactic disk. No obvious spiral arm structures are visible. The galaxy does not exhibit any prominent tidal features or signs of ongoing major mergers, although subtle asymmetry in the outer regions hints at a possible minor interaction. The overall shape appears more or less round, rather than elongated. The mass of the galaxy is likely substantial.
