The galaxy presents as a moderately bright, lenticular or early-type spiral galaxy with a smooth, centrally concentrated light distribution. The overall shape appears elliptical, with a high degree of roundness, and a lack of any obvious spiral arm structures or significant dust lanes. The color profile suggests a dominant population of older stars, indicated by the yellowish-red hue, particularly concentrated toward the galactic center. There is some evidence of a faint, blueish halo surrounding the central bulge, suggesting the presence of some younger stars. The galaxy does not appear to be undergoing any major merger events or show significant signs of tidal disturbance.
