This galaxy presents as a moderately luminous object with a distinct, elongated morphology. The galaxy exhibits a noticeable degree of central concentration, gradually fading towards its periphery. The central region appears relatively smooth and uniform in color, suggesting an older stellar population.

There is a visible disk-like component, although it appears somewhat disturbed or warped. Possible merger activity is inferred by the galaxy's asymmetrical form and potential tidal features, appearing as faint extensions or distortions in the outer regions. The redder color suggests that there is substantial presence of dust lanes.
