The galaxy appears to be an elliptical type, exhibiting a smooth, spheroidal morphology with a relatively high degree of roundness. The galaxy’s color profile suggests a population of older stars, with a dominant redder hue indicating lower levels of ongoing star formation. There is some evidence of a possible minor interaction, as subtle disturbances appear to be present in its overall structure. The estimated physical size suggests a moderate extent. There may be a merger in progress as well.