The galaxy presents as an elliptical morphology with a smooth, diffuse light distribution and minimal discernible features. Its shape appears slightly elongated rather than perfectly spherical. The central region exhibits a concentrated luminosity, transitioning outwards to fainter, more diffuse edges. Color analysis reveals a dominant yellowish-orange hue, suggesting a relatively older stellar population with suppressed ongoing star formation. There is a subtle hint of bluer light at the extreme outer edges, possibly indicative of recent or ongoing star formation at very low levels. No obvious signs of spiral arms, dust lanes, or tidal disturbances are apparent. There is no indication of an active galactic nucleus. The galaxy seems to be relatively isolated.
