The galaxy presents a generally smooth appearance, with a subtle disk-like structure subtly apparent. There is a slight elongation, suggesting it is not perfectly spherical but more along the lines of cigar-shaped. The central bulge exhibits a concentrated, bright yellowish hue. There's no strong evidence of recent or ongoing major mergers, although there may be a minor disturbance that could be from a gravitational interaction. The color profile indicates a relatively mature stellar population, consistent with a galaxy where star formation has slowed, but is still active. The overall luminosity suggests a fairly massive galaxy.
