The galaxy presents as a relatively smooth object with a concentrated central bulge. The overall color appears reddish, indicating a population of older stars and a potentially lower rate of ongoing star formation. The shape is approximately elliptical, showing no clear spiral arm structure or significant disk features. The galaxy's light profile suggests a centrally concentrated mass distribution. There are no obvious signs of a major ongoing merger, although subtle disturbances cannot be entirely ruled out. The overall morphology aligns with that of an elliptical galaxy exhibiting characteristics of an older stellar population with a redshift of approximately 0.25.