This galaxy exhibits a generally smooth morphology, with no immediately apparent spiral arm structures or significant dust lanes. The overall shape is somewhat elongated, approximating a cigar shape, which suggests it may be an elliptical galaxy or a lenticular galaxy seen edge-on or at a high inclination. There appears to be a concentration of light toward the center, indicative of a galactic bulge. The color profile shows a tendency towards redder hues, hinting at an older stellar population and a potentially lower ongoing star formation rate. There is no strong evidence of any major merging activity or significant tidal disturbances in the immediate vicinity of the galaxy. The galaxy is of intermediate size.
