The galaxy appears as a relatively smooth, elliptical-like structure. The light is concentrated towards the center, indicating a dense galactic nucleus. The color profile suggests a predominantly older stellar population, with a yellowish-red hue. This, combined with the smoothness, implies that the galaxy is likely an early-type galaxy, possibly an elliptical or lenticular galaxy undergoing little to no active star formation at present. There is no evidence of spiral arms, significant dust lanes, or major disturbances, supporting the assessment of a non-merging system. The galaxy exhibits a moderate angular size, suggesting an intermediate distance. The light is generally uniformly distributed, and while there are some irregularities in the very faint light, there is no evidence of very distinct features beyond the primary spheroid shape.