The galaxy presents as an elliptical morphology, appearing as a diffuse, elongated spheroid with a smooth light distribution. Its major axis is oriented at approximately 45 degrees relative to the image frame. There is a notable concentration of light toward the center, suggesting a dense core or nucleus. The galaxy exhibits a yellow-reddish hue, indicative of an older stellar population dominated by evolved stars. There is no clear evidence of spiral arms or distinct features indicative of active star formation, such as blue knots or dust lanes. A slight asymmetry or minor disturbance cannot be completely ruled out due to the slight fuzziness in the image. The galaxy appears relatively isolated, showing no immediate signs of ongoing major merger activity.
