This galaxy appears to be an elliptical or lenticular type, characterized by a generally smooth and featureless morphology. It exhibits a concentrated central bulge, with luminosity gradually decreasing towards the outer regions. The color profile suggests a population of older stars, evidenced by the yellowish-orange hue, indicating lower levels of current star formation. There are subtle hints of disturbances or minor interactions, based on slight irregularities in the outer halo. The overall impression is of a galaxy with a moderate stellar mass and a relatively low specific star formation rate.
