The galaxy presents as a somewhat elliptical object, exhibiting a relatively smooth and concentrated central bulge. There's a notable lack of distinct spiral arm structure. The color profile suggests an older stellar population, leaning towards redder hues overall, with bluer tints concentrated within the central region. Evidences of merging or major disturbances appear minimal, although there is some irregular structure present. The galaxy appears relatively isolated with no obvious interactions with nearby objects. The luminosity indicates an absolute magnitude somewhere in the range of -18 to -19. The morphology seems to trend towards a relatively smooth galaxy that is also rather round in shape.
