The galaxy presents as a centrally concentrated object with a generally smooth appearance. It exhibits a somewhat elliptical morphology, appearing more elongated than perfectly spherical. The core region of the galaxy is characterized by a bright, yellowish hue, suggesting a concentration of older stellar populations. Progressing outwards from the core, the color gradually shifts towards bluer tones in the surrounding areas, potentially indicating the presence of younger, hotter stars. There is no apparent spiral structure or bar feature. No obvious signs of tidal disturbance or interaction with other galaxies are observed. The overall morphology suggests this is likely an early-type galaxy, potentially an elliptical or lenticular galaxy, at an approximate distance that implies significant luminosity. The presence of bluer colors in the outer regions may point to ongoing, albeit possibly low-level, star formation activity.
