The galaxy presents an overall smooth morphology, suggesting it may be an elliptical galaxy. The central region exhibits a high concentration of light, appearing bright and somewhat spherical. A fainter, extended halo surrounds the core, contributing to a diffuse overall appearance. There are no distinct spiral arms or well-defined dust lanes visible. The color index appears slightly redder, consistent with a population of older stars. The galaxy is not perfectly spherical, showing a slight elongation along its major axis, and perhaps shows some minor signs of disturbance or interaction, with a subtle, irregular extension on one side, which may be a sign of a past merger event. Some clumps of light are observed throughout the galaxy that may be merging galaxies, further reinforcing the idea of a past merger. 