The galaxy appears as a smooth, elongated structure, indicative of an elliptical morphology. The central region exhibits a bright, concentrated core. The color profile suggests a population of older stars, with a yellowish to reddish hue dominating. There is little evidence of distinct spiral arms or significant dust lanes. Overall the galaxy does not appear to be experiencing significant ongoing star formation. The shape is consistent with a spheroidal system, but it seems to be more elongated than perfectly round. There is a slight suggestion of possible tidal features or minor disturbances, but the resolution limits conclusive identification. There are no apparent signs of an actively merging system.
