The galaxy appears as a centrally concentrated, elliptical-like object with a relatively smooth light distribution. The core region exhibits a high degree of luminosity, gradually decreasing towards the outer edges. The morphology suggests it may be an early-type galaxy. A slight elongation is visible, indicating a non-spherical shape, possibly an oblate spheroid. There is no clear evidence of spiral arms, dust lanes, or significant star-forming regions within the galaxy from this image. The overall color seems to be somewhat yellowish or white, consistent with a population of older stars and a lower rate of star formation. No prominent tidal features or indications of a recent major merger event are evident. There is a faint, diffuse halo extending beyond the bright central region.
