The galaxy presents as a moderately bright object with an overall smooth appearance, with a noticeable central bulge. The color distribution indicates a predominantly older stellar population, displaying a yellow-orange hue in the core region. A faint hint of bluer light is visible peripherally, suggesting the presence of some younger, hotter stars, although this is not a dominant feature. The galaxy appears relatively round. There are potential signs of gravitational interaction, possibly in the form of tidal tails or distortions, though these features are faint and uncertain. A possible merger is either in progress or recently completed.
