The galaxy presents as a slightly elongated, lenticular structure. The color profile suggests an older stellar population, predominantly exhibiting reddish-yellow hues. The morphology indicates a relatively smooth distribution of light, with a possible disk-like component. The galaxy does not show any strong evidence of ongoing star formation. There is a slight asymmetry to the galaxy, but no obvious major disturbances are seen to suggest a merger event. There is a slight hint of a tidal feature, but nothing significant enough to confirm a major interaction.
