The galaxy appears to be an elliptical galaxy, characterized by a smooth, featureless morphology. It exhibits an elongated shape, tending towards a cigar-like appearance rather than a perfectly circular form. The light distribution shows a concentration towards the center, indicating a dense core. The color gradient is subtle, with a yellowish-white core possibly suggesting an older stellar population. The outer regions appear redder, which could be due to dust absorption or a slightly younger stellar population compared to the core. There is no evidence of spiral arms or significant star formation regions visible within the galaxy based on the color or morphology. The galaxy is relatively isolated, without any obvious signs of recent mergers or major tidal disturbances. The lack of blue color suggests that star formation is suppressed.