The galaxy presents as a slightly elliptical or spheroidal structure, with a centrally concentrated luminosity profile. The core region is characterized by a high surface brightness, suggesting a dense concentration of stars. Moving outward from the core, the luminosity gradually decreases, blending into a fainter, more diffuse halo.

There's a hint of some features or disk-like structures within the galaxy, but it is difficult to confirm from the data. There is also no evidence of strong spiral arm structures or a distinct bar feature. The galaxy exhibits a smooth appearance, with some irregularities or disturbances, perhaps indicative of past or ongoing interactions. Given its overall morphology and color profile, the galaxy appears to be a moderately massive system with an active star formation rate.
