The galaxy presents as a relatively smooth and centrally concentrated object, likely an elliptical galaxy, though the possibility of a highly inclined spiral disk cannot be entirely excluded with this image alone. It appears moderately luminous in the observed bands. The galaxy does not display any strong spiral arm structures, although it is slightly elongated. There's some indication of minor disturbance in the symmetry or light distribution, however, this could also be an artifact of the image. The color profile appears relatively uniform across the galaxy body, with a generally redder hue that suggests a population of older stars. Star formation rates appear low. The galaxy's apparent size is small, suggesting it's either intrinsically compact or at a substantial distance. The presence of what looks like a tidal tail or disturbance suggests it is currently, or recently, in the process of merging with another object.
