The galaxy appears to be an elliptical galaxy, possibly of type E4-E5, displaying a moderately flattened shape, as observed from our vantage point. Its light distribution suggests a largely smooth morphology, with no readily discernible spiral arms or significant disk structure. The color profile indicates a population of older stars, which is consistent with the overall reddish hue and lack of prominent blue star-forming regions. There is no apparent tidal debris or other indications of a recent major merger event, although subtle asymmetries might suggest minor gravitational interactions. The galaxy's size is typical for an elliptical at its estimated distance, neither exceptionally large nor compact.
