The galaxy exhibits a generally smooth morphology, with a largely featureless appearance, suggesting it may be an elliptical or lenticular type. The core of the galaxy appears bright and concentrated, gradually fading outwards into a diffuse halo. There is a slight elongation, though the galaxy is generally quite round. The color profile suggests an older stellar population. A faint greenish color indicates some star formation is possible, though generally the color is much redder, indicating a population of older, redder stars dominates. There is no obvious indication of recent or ongoing major mergers or tidal interactions. The faintness of the outer regions relative to the bright core is suggestive of a galaxy with relatively low star formation activity.
