This galaxy presents an elongated morphology, displaying characteristics indicative of a potential ongoing or recent interaction or merging event. The primary body of the galaxy exhibits a relatively smooth, unresolved structure, with a central, bright region suggesting a higher concentration of stellar density, possibly a bulge. A distinct extension or tidal tail is observed extending from this central region, characterized by a redder hue suggesting an older stellar population.

The overall color profile suggests a mixed stellar population, with the central body potentially hosting younger, bluer stars alongside older, redder stars evident in the tail. The smoothness of the primary body is contrasted by the disrupted appearance implied by the tail, leading to the conclusion of a significant gravitational disturbance. This galaxy's absolute magnitude suggests it is a fairly luminous object. The estimated mass of the galaxy is substantial, typical of large galaxies. The rate of star formation is low compared to other galaxies of a similar mass.
