The galaxy presents an elliptical morphology, appearing somewhat flattened in shape. The central region is characterized by a bright, concentrated luminosity, suggesting a high stellar density, possibly containing an older stellar population. Moving outwards from the core, the luminosity gradually decreases. The outer regions display a bluer hue than the central bulge, hinting at the presence of younger, hotter stars and potentially ongoing star formation activity, although the galaxy appears relatively smooth with few distinct features beyond its overall shape and color gradient. There is a slight asymmetry or minor disturbance that can be seen as the even luminosity and structure of the disk is not perfect, perhaps due to the interaction with another galaxy. Overall, the galaxy is moderately sized and has a redshift of about 0.147.
