This galaxy exhibits a relatively smooth morphology, with a dominant central bulge. The light is concentrated towards the core, suggesting a higher density of older stellar populations in that region. The galaxy appears to have an elliptical shape, possibly exhibiting a slight disk-like structure, although it is not well defined. There is some irregularity in the outer regions. Subtle hints of spiral arms, or potentially tidal streams, may be present. There's a possible interaction or minor disturbance in the galaxy's overall form. Its color indicates moderate star formation activity. The galaxy's reddish hue suggests a population of evolved stars.
