The galaxy presents as a largely smooth, elliptical-like structure. The central region exhibits a concentrated, yellowish-white luminosity, suggesting an older stellar population is dominant in the core. Fainter, bluer light surrounds this core, which could indicate the presence of a younger stellar population or ongoing star formation activity at the outskirts. There are no distinct spiral arms, bars, or dust lanes visible within the galaxy's structure. The overall shape appears generally rounded, with no significant morphological disturbances or signs of ongoing mergers, though some minor irregularities may be present. The galaxy exhibits a moderate degree of spatial extent, implying it is a reasonably large system.
