The galaxy presents as an elliptical morphology, exhibiting a smooth, concentrated light profile indicative of an early-type system. The light distribution appears largely homogenous without prominent spiral arms or distinct features like dust lanes. The central region of the galaxy demonstrates a slightly higher concentration of light, suggesting the presence of a galactic nucleus. The overall color index suggests a population of older stars, with a relatively low rate of current star formation activity. There is no evidence of ongoing merger activity or major tidal disturbances within the immediate vicinity of the galaxy.