The galaxy appears to be an elliptical galaxy, exhibiting a generally smooth and round morphology. There is a notable absence of spiral arms or significant dust lanes. The galaxy presents a concentrated central bulge that fades into the outer regions. The color profile suggests an older stellar population with a yellowish to reddish hue, indicative of a galaxy where star formation has substantially decreased. There is no evidence of tidal tails or major distortions in the galaxy's structure that would indicate a recent major merger event, though subtle disturbances cannot be ruled out.
