The galaxy presents as a somewhat luminous, elliptical structure. It has a smooth and concentrated central bulge, suggesting an older stellar population. The galaxy exhibits a faint disk component, inclined relative to our line of sight, evident through some asymmetrical dust and star formations. Notably, there appears to be a disturbance or merging event occurring on one side of the galaxy, marked by a distinct reddish plume. The plume suggests ongoing star formation. Overall, the galaxy appears to be in transition, showing characteristics of both early-type and late-type galaxies, possibly due to an interaction.