This galaxy exhibits an overall smooth morphology, with a slight elongation. There is a dominant central bulge characterized by a yellowish-orange hue, possibly indicating an older stellar population. The galaxy does not possess well-defined spiral arms, but there appear to be some faint disk-like features or minor disturbances extending from the core region. There is some possible evidence of interactions with companion galaxies. The overall form suggests a galaxy transitioning between a spiral and elliptical morphology. The galaxy displays a range of colors, from the bluer regions suggesting younger stellar populations, to redder and yellower areas associated with aging stars and dust.
