This galaxy presents as a concentrated, centrally-bright object. It exhibits a generally smooth morphology with a near-circular appearance in the observed image. The light distribution is concentrated with a radial falloff of intensity. There is no indication of spiral arms, bar structures, or a well-defined disk. A slight elongation is barely perceptible. The galaxy exhibits a yellow hue, indicating a population of older stars and a lower rate of ongoing star formation. There might be very slight evidence of a minor gravitational interaction, showing some distortion.
