The galaxy presents as an elliptical or lenticular morphology, exhibiting a relatively smooth overall appearance. Its core appears to be bright and concentrated, suggesting a higher density of older stellar populations. A less concentrated, bluer area extends perpendicular from the core. Some of this region appears diffuse, possibly indicating ongoing star formation activity. The overall shape leans toward slightly elongated, though not significantly cigar-shaped. There are some features suggesting the presence of a recent or ongoing merger event. The galaxy exhibits noticeable tidal features that hint at interactions with another galaxy, even if there is only minor disturbance.
