The galaxy exhibits an overall elliptical morphology, appearing mostly smooth and spheroidal. The central region displays a concentrated luminosity gradient, suggesting a dense stellar population within the galactic nucleus. Moving outward from the center, the light intensity gradually diminishes. The color profile indicates a redder hue in the core, potentially indicative of older stellar populations and/or dust obscuration. The outer regions show a slight bluer tint, suggesting the presence of a younger population of stars, though still subtle. The major to minor axis ratio suggests it is moderately elliptical. No prominent spiral arms, bars, or tidal features are discernible. The overall appearance points towards an early-type galaxy, potentially an elliptical or lenticular galaxy, displaying a mature stellar population with suppressed star formation.
