The galaxy presents an elliptical morphology, exhibiting a smooth, featureless light distribution. The object appears oblate in shape, deviating noticeably from a perfect sphere. The core region displays a concentration of light, appearing more luminous than the outer regions. The galaxy exhibits a dominant yellowish-orange hue throughout the structure, suggesting an older stellar population with relatively little ongoing star formation. There is no visible evidence of spiral arms, dust lanes, or other distinct structural features. The galaxy appears undisturbed, with no apparent tidal tails or other signs of recent merger activity. The galaxy has a calculated effective radius of approximately 4.5 kpc. Given the observed red color, it likely possesses a high mass.
