The galaxy presents as a centrally concentrated, elliptical morphology. A bright, yellowish core dominates the structure, suggesting an older stellar population. The light profile appears smooth and decreases steadily away from the nucleus, with no distinct spiral arm features or obvious dust lanes visible. A slight elongation is noted, though the overall shape is largely spheroidal. There is no evidence of ongoing major mergers or significant tidal disturbances based on current imaging. The galaxy appears relatively isolated and undisturbed. The observed color suggests a relatively low star formation rate.
