The galaxy exhibits a somewhat elliptical morphology, with an estimated physical size of approximately 4 kpc in radius. It appears relatively smooth in structure, lacking any immediately obvious spiral arms or a prominent central bar. There's a central bulge region which has a bright, concentrated luminosity, with intensity diminishing outwards. The galaxy's color profile suggests a mix of stellar populations, with redder hues toward the center indicating older stars or a higher dust content, contrasting with bluer regions that may indicate ongoing star formation. The overall light distribution appears well-defined, the object is likely early-type or intermediate disk galaxy with a slight ellipticity. Furthermore, the overall appearance suggests that a merger may be underway, indicated by the irregular light distribution towards the outer edges.
