The galaxy presents as a slightly elliptical structure, exhibiting a smooth, centralized bulge dominating the overall light distribution. The core of the galaxy appears to be a concentrated source of light, potentially indicating the presence of an active galactic nucleus or a region of intense star formation. Moving outward from the center, the light distribution gradually diminishes, suggesting a spheroidal or elliptical morphology. A faint disk may be present, but difficult to distinguish. The colors suggest a mix of stellar populations, with the redder hues potentially indicative of older, cooler stars and/or dust obscuration, while the bluer colors could represent younger, hotter stars. There is no obvious evidence of spiral arms or a complex disk structure. The galaxy appears relatively isolated, without any prominent signs of tidal interactions or ongoing mergers.