The galaxy appears to be an elliptical or lenticular type, exhibiting a generally smooth morphology with a concentrated central bulge. A subtle disk-like structure may be present but is not distinctly defined. The galaxy's color profile suggests a population of primarily older stars, exhibiting a redder overall hue with some younger blue stars visible. There's no strong evidence of recent major merging activity, though there is some asymmetry. Star formation is likely low within the system, as indicated by the lack of bright HII regions. The galaxy is moderately luminous and has a substantial mass.
