This galaxy presents as a relatively smooth, centrally concentrated object with a slight elongation. The core region exhibits a bright, yellowish hue, suggesting an older stellar population. There is a gradual decrease in luminosity from the center outwards. The overall color profile indicates that it is relatively red, possibly due to dust extinction or a population of older stars. The galaxy displays a faint blue disk-like morphology, with an absence of distinct spiral arms or prominent dust lanes. There is a suggestion of a minor disturbance or interaction visible, but it would need more imaging to confirm.
