The galaxy presents an elliptical morphology, elongated along its major axis. The central region exhibits a concentrated, bright core, indicative of a substantial stellar population. Moving outward from the core, the luminosity gradually decreases. The galaxy displays a smooth overall texture, suggesting a relatively older stellar population with less active star formation. There are no obvious spiral arm structures or prominent dust lanes visible in this image. The color profile appears to be redder in the central regions, possibly due to the presence of older, redder stars or dust obscuration. Fainter blue regions can be seen, suggesting some small areas of recent star formation. The galaxy appears relatively undisturbed, without any major signs of mergers or tidal interactions.
