This galaxy appears to be a relatively bright, massive system at a considerable distance, with an estimated redshift of approximately 0.24. It exhibits a generally smooth morphology, with a somewhat elliptical shape, though some minor disturbances are suggested. The light distribution indicates a higher concentration of older stars toward the center, with a distinct color gradient extending outwards. There is likely a modest amount of ongoing star formation, as evidenced by the less prominent bluer regions in the outer regions. The outer parts of the galaxy show some clumpy features, possibly indicating tidal debris or recent minor merger activity. The galaxy's overall structure seems reasonably intact, indicating that any interactions are not overly disruptive to its global form.
