The galaxy presents an elliptical morphology, displaying a smooth, featureless light distribution without prominent spiral arms or a distinct disk. The object exhibits an elongated shape. The color profile indicates a reddish hue, suggesting a population dominated by older stars and a relatively low rate of ongoing star formation. There is some indication of possible tidal disturbance or interaction with another galaxy based on the extended light and slightly irregular shape, although a clear merger is not evident. The galaxy appears relatively massive and luminous, consistent with a large population of stars.
