The galaxy appears as a moderately luminous, spatially resolved object. It exhibits a generally smooth morphology, with a concentrated central region. The light profile suggests a gradual decline in surface brightness from the core outwards, with no apparent spiral arm structures or distinct features typically associated with disk galaxies. The color distribution shows a yellowish central region, possibly indicative of an older stellar population, gradually transitioning to a redder hue in the outer regions. There might be some subtle asymmetry in the outer isophotes, potentially hinting at a minor interaction or disturbance. The galaxy's overall shape is more elliptical than circular, suggesting a spheroid-dominated system. No signs of active star formation regions or prominent dust lanes are visible in the current image resolution and color bands.
