The galaxy presents as a slightly elongated, lenticular-like structure. Its core appears to be a bright yellowish-white, suggesting a significant population of older stars. The light tapers off smoothly from the center, with no distinct spiral arms or features immediately apparent. There's a subtle color gradient, shifting towards a slightly redder hue in the outer regions. This could indicate either the presence of older stellar populations or dust lanes attenuating bluer light. Overall, the galaxy exhibits a high degree of smoothness and a lack of strong irregularities. There is slight asymmetry. A faint, irregular, redder area appears on the upper left of the galaxy. This could be a star formation region or evidence of a minor gravitational interaction. The galaxy appears relatively isolated, with no obvious signs of major merger activity.
