The galaxy presents as a somewhat elongated, diffuse object. It exhibits a smooth, centrally concentrated luminosity profile, with the light appearing brightest near the center, gradually fading towards the edges. The galaxy's apparent shape is neither perfectly spherical nor highly flattened; it could be considered moderately elliptical. There are faint hints of disturbance in the outer regions of the galaxy, with one side appearing more irregular than the other. The galaxy appears to be primarily composed of older stellar populations, indicated by its redder color, although some bluer patches are visible towards the galaxy's center. The presence of these bluer regions suggests the possibility of ongoing, albeit low-level, star formation within the galaxy's core. Overall, it has an estimated size of 5.1 Kpc, and a redshift of approximately 0.088, placing it at a considerable distance.
