The galaxy appears as an elliptical or lenticular system, exhibiting a generally smooth light distribution. Its central region presents a yellowish-white hue, indicative of an older stellar population, potentially dominated by evolved stars. Moving outward from the core, the galaxy's color transitions towards a bluer periphery, suggesting the presence of younger stars or ongoing star formation, albeit at a relatively low rate, in its outer regions. The galaxy's overall shape is elongated, lacking any clear spiral arm structure or prominent disk features. There is also a suggestion of some minor gravitational disturbance, though the overall symmetry is not greatly disrupted. The size of the galaxy is of a moderate size.