The galaxy presents as a somewhat elliptical structure, with a brighter, concentrated central bulge. The color profile appears yellow-orange in the central region, suggesting a population of older stars. The outer regions show a gradual fading in intensity and a slight bluer tint compared to the core, hinting at the presence of younger stars and possibly some ongoing star formation within a weak or obscured disc structure. The galaxy exhibits a relatively smooth appearance, with no strong indication of spiral arms or prominent dust lanes visible. The overall form could be described as an early-type spiral or perhaps an elliptical galaxy with a residual disc.
