The galaxy presents as a somewhat elliptical structure, exhibiting a noticeable central bulge that appears to be a dominant feature. The light distribution suggests a higher concentration of older stars in the central region, likely contributing to the bulge's yellowish-orange hue. Moving outwards from the core, the galaxy seems to fade into a less distinct halo. The overall color profile indicates a relatively passive galaxy, potentially with a low rate of ongoing star formation. There are no clearly visible spiral arm structures or other pronounced features, suggesting a morphology that is more characteristic of an early-type galaxy. A slight deviation from a perfectly circular shape is observed, indicating that it is more of a flat ellipse than a circle. The galaxy appears relatively isolated, with no immediate signs of tidal disruption or close interaction with other large systems in the immediate vicinity.
