The galaxy presents a generally smooth morphology, but with a discernible feature extending from the primary body. The galaxy exhibits a central concentration of light, appearing yellowish-white, suggesting an older stellar population. This central region appears fairly circular. Extending from this core is a less defined region that seems to be undergoing some form of interaction, perhaps with an area of increased star formation that is bluer in color. The galaxy appears relatively undisturbed despite this interaction, and its primary structure remains largely intact. Based on the color index, it may be of an early type. The galaxy shows characteristics of a possible merging event in its overall structure, although it isn't exhibiting signs of significant disruption.
