The galaxy presents as a centrally concentrated object with a mostly smooth appearance. The central region exhibits a yellowish hue, suggesting an older stellar population. Surrounding the core is a more diffuse, bluish halo, hinting at the presence of younger, hotter stars or potential star-forming regions. There appears to be a slight asymmetry or minor disturbance in the outer regions of the galaxy, possibly indicative of a past or ongoing minor interaction. The overall shape approximates a rounded form but with slight irregularities. The galaxy does not exhibit a clearly defined spiral structure or a prominent disk component.
