The galaxy presents as a predominantly smooth, elliptical morphology. The core region exhibits a high concentration of light, appearing bright and somewhat unresolved in this imaging. Moving outward from the core, the light intensity decreases gradually. The galaxy lacks distinct spiral arm structures or other prominent features typically associated with disk galaxies. There is a suggestion of a very slight disturbance on the outer edges of the galaxy, with possibly a faint tidal tail pointing away from the central core. Overall, the galaxy's structure indicates an older stellar population and the absence of significant ongoing star formation. The galaxy's color suggests it is relatively red, which is consistent with a lack of active star formation and the presence of older, redder stars.
