The galaxy exhibits a generally elliptical morphology. It has a diffuse, centrally concentrated bulge that is tinged yellow. The light distribution appears relatively smooth across the galaxy, with some suggestion of a fainter, less defined disk structure extending beyond the central bulge region. There is evidence of some possible disturbances, such as faint tidal features that disrupt the light profile around the central region. The color profile suggests ongoing star formation, potentially at a rate which is not very high. The galaxy does not appear to be undergoing a major merger, but may be experiencing or have recently experienced a minor interaction. The galaxy appears relatively isolated. Overall, the galaxy presents as an intermediate-mass system with a mixture of old and young stellar populations.