The galaxy presents as a moderately bright, extended object with an elliptical morphology. The central region exhibits a relatively smooth and concentrated light distribution, indicative of a bulge component. Moving outward from the center, the light appears to gradually diminish with some disturbances. The overall shape is somewhat rounded, but with some apparent asymmetries suggesting potential tidal interactions or mergers. There is evidence of faint, extended features that could be interpreted as tidal tails or disrupted spiral arms, hinting at past or ongoing gravitational interactions. The galaxy's colour profile suggests a stellar population that may be somewhat evolved.
